ASA UWF300 f1.3 + DDM100 + wedge
One of the fastest telescopes of the world!
The UWF300_1 package combines the highly-corrected 300mm f1.3 UWF OTA with our outstanding ASA DDM100 mount. This groundbreaking optical design is ideal for short exposure, high SNR wide field surveys.
The main mirror works with absolute encoder feedback and can be collimated fully electronic for an easy and fast remote collimation.
The DDM100 Direct Drive mount is a precision platform ready for fully automated imaging.
Main Facts
Ultra Wide Field, prime corrector
51%
390mm
f1.3
300mm (11.8 inch) / f1.3
52mm (7.58 degrees)
Fused silica
<7um RMS
>80 strehl
1.3nm RMS / <0.7nm Ra
Al+SiO2 >96%
25.14mm
30kg (66lbs) (no camera or filter)
ASA Direct Drive
0 to 90 degrees
56kg (123lbs)
ASA Software package with a platform-independent Ascom Alpaca API (via TCP/IP), compatibility with numerous programs, and many additional API features for:
• Creating and optimizing pointing files
• MLPT (e.g., usable with a N.I.N.A plugin)
• Uploading and tracking TLE and CPF satellite orbits
• Orbit corrections when satellite tracking (autoguiding with external CCD cameras)
• Focus control also via Ascom Alpaca API
• Covers (if installed) via Ascom Alpaca API
Up to 50 degrees per second
<8” RMS with pointing model
<0,25” RMS within 5 minutes
10 Hz or greater
Technical Details
Our closed loop direct drive systems, sensor technology and observatory safety modules play a major role in achieving optimum results. All moving accessory components are equipped with high-resolution encoders and closed-loop feedback systems. We provide event timer modules, and customer updatable firmware.
ASA In-house production
The competent partner that provides you with the whole package – ASA, guarantees the highest standard! Interferometric metrology, CNC machining, meter class optics, light weight mirrors, telescope systems, ground stations, assembly, factory testing and commissioning, everything is done by ASA itself.
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